Spherically Symmetric Gravitational Collapse
arXiv:0812.0646 · doi:10.1142/S0217732309030072
Abstract
In this paper, we discuss gravitational collapse of spherically symmetric spacetimes. We derive a general formalism by taking two arbitrary spherically symmetric spacetimes with . Israel's junction conditions are used to develop this formalism. The formulae for extrinsic curvature tensor are obtained. The general form of the surface energy-momentum tensor depending on extrinsic curvature tensor components is derived. This leads us to the surface energy density and the tangential pressure. The formalism is applied to two known spherically symmetric spacetimes. The results obtained show the regions for the collapse and expansion of the shell.
12 pages, 4 figures, accepted for publication in Mod. Phys. Lett. A
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- Expanding and Collapsing Scalar Field Thin Shell
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- Spherical Symmetric Gravitational Collapse in Chern-Simon Modified Gravity
- Dynamical model of expansion free dissipative perfect fluids in general relativity